Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Rin I. Yamada"'
Autor:
Kazuyuki Muraoka, AAS Journals Data Editors, Ayu Konishi, Kazuki Tokuda, Hiroshi Kondo, Rie E. Miura, Tomoka Tosaki, Sachiko Onodera, Nario Kuno, Masato I. N. Kobayashi, Kisetsu Tsuge, Hidetoshi Sano, Naoya Kitano, Shinji Fujita, Atsushi Nishimura, Toshikazu Onishi, Kazuya Saigo, Rin I. Yamada, Fumika Demachi, Kengo Tachihara, Yasuo Fukui, Akiko Kawamura
Publikováno v:
The Astrophysical Journal, Vol 953, Iss 2, p 164 (2023)
We present the results of ALMA-ACA 7 m array observations in ^12 CO( J = 2–1), ^13 CO( J = 2–1), and C ^18 O( J = 2–1) line emission toward the molecular-gas disk in the Local Group spiral galaxy M33 at an angular resolution of 7.″31 × 6.″
Externí odkaz:
https://doaj.org/article/d268689c85164dbca3b678c3e93a8777
Autor:
Mikito Kohno, James O Chibueze, Ross A Burns, Toshihiro Omodaka, Toshihiro Handa, Takeru Murase, Rin I Yamada, Takumi Nagayama, Makoto Nakano, Kazuyoshi Sunada, Kengo Tachihara, Yasuo Fukui
Publikováno v:
Publications of the Astronomical Society of Japan. 75:397-415
We have carried out the NH$_3$ $(J,K)=(1,1),(2,2),$ and $(3,3)$ mapping observations toward the Galactic infrared bubble N49 (G28.83-0.25) using the Nobeyama 45 m telescope. Three NH$_3$ clumps (A, B, and C) were discovered along the molecular filame
Autor:
Rin I Yamada, Yasuo Fukui, Hidetoshi Sano, Kengo Tachihara, John H Bieging, Rei Enokiya, Atsushi Nishimura, Shinij Fujita, Mikito Kohno, Kisetsu Tsuge
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 515:1012-1025
We have carried out a new kinematical analysis of the molecular gas in the Sh2-233 region by using the CO $J$ = 2-1 data taken at $\sim$0.5 pc resolution. The molecular gas consists of a filamentary cloud of 5-pc length with 1.5-pc width where two de
Autor:
Mikito Kohno, Toshihiro Omodaka, Toshihiro Handa, James O Chibueze, Takumi Nagayama, Ross A Burns, Takeru Murase, Ren Matsusaka, Makoto Nakano, Kazuyoshi Sunada, Rin I Yamada, John H Bieging
Publikováno v:
Publications of the Astronomical Society of Japan. 74:545-556
We performed NH$_3\ (J,K)=(1,1),(2,2),$ and $(3,3)$ mapping observations toward the Galactic massive star-forming region Sh 2-255 and Sh 2-257 using the Nobeyama 45-m telescope as a part of the KAGONMA (KAgoshima Galactic Object survey with the Nobey